Matches in SemOpenAlex for { <https://semopenalex.org/work/W2034333708> ?p ?o ?g. }
- W2034333708 endingPage "176" @default.
- W2034333708 startingPage "165" @default.
- W2034333708 abstract "We have thoroughly characterized the ultraviolet to near-infrared (0.15 - 2.2 micron) spectral energy distribution (SED) of the central parsec of the M33 nucleus through new infrared photometry and optical/near-infrared spectroscopy, combined with ultraviolet/optical observations from the literature and the HST archive. The SED shows evidence for a significant level of attenuation, which we model through a Monte Carlo radiative transfer code as a shell of clumpy Milky Way-type dust (tau_V ~ 2 +/- 1). The discovery of Milky Way-type dust (with a strong 2175 A bump) internal to the M33 nucleus is different from previous work which has found SMC-like dust (no bump) near starburst regions. The amount by which dust can be processed may be related to the mass and age of the starburst as well as the extent to which the dust can shield itself. Our starburst models include the effects of this dust and can fit the SED if the nucleus was the site of a moderate (~10^8 L_sun at 10 Myrs) episode of coeval star formation about 70 Myrs ago. This result is quite different from previous studies which resorted to multiple stellar populations (between 2 and 7) attenuated by either no or very little internal dust. The M33 nuclear starburst is remarkably similar to an older version (70 Myr versus 10 Myr) of the ultra-compact starburst in the center of the Milky Way." @default.
- W2034333708 created "2016-06-24" @default.
- W2034333708 creator A5000945647 @default.
- W2034333708 creator A5012069547 @default.
- W2034333708 creator A5029607045 @default.
- W2034333708 creator A5051018099 @default.
- W2034333708 creator A5089400895 @default.
- W2034333708 date "1999-07-01" @default.
- W2034333708 modified "2023-09-25" @default.
- W2034333708 title "The Dusty Starburst Nucleus of M33" @default.
- W2034333708 cites W1611483743 @default.
- W2034333708 cites W1920718865 @default.
- W2034333708 cites W1964172655 @default.
- W2034333708 cites W1971863221 @default.
- W2034333708 cites W1974174849 @default.
- W2034333708 cites W1980842862 @default.
- W2034333708 cites W1981222868 @default.
- W2034333708 cites W1984139715 @default.
- W2034333708 cites W1987146716 @default.
- W2034333708 cites W1987532627 @default.
- W2034333708 cites W1992061927 @default.
- W2034333708 cites W1999488682 @default.
- W2034333708 cites W2003858398 @default.
- W2034333708 cites W2004795388 @default.
- W2034333708 cites W2006360799 @default.
- W2034333708 cites W2013594775 @default.
- W2034333708 cites W2014051283 @default.
- W2034333708 cites W2014841467 @default.
- W2034333708 cites W2015295900 @default.
- W2034333708 cites W2016911950 @default.
- W2034333708 cites W2018643625 @default.
- W2034333708 cites W2019103771 @default.
- W2034333708 cites W2020203444 @default.
- W2034333708 cites W2026795906 @default.
- W2034333708 cites W2028468856 @default.
- W2034333708 cites W2033835256 @default.
- W2034333708 cites W2042738789 @default.
- W2034333708 cites W2048756914 @default.
- W2034333708 cites W2051920470 @default.
- W2034333708 cites W2061959687 @default.
- W2034333708 cites W2063343513 @default.
- W2034333708 cites W2073334118 @default.
- W2034333708 cites W2083845016 @default.
- W2034333708 cites W2088093732 @default.
- W2034333708 cites W2088853013 @default.
- W2034333708 cites W2092445825 @default.
- W2034333708 cites W2093172397 @default.
- W2034333708 cites W2093911390 @default.
- W2034333708 cites W2135615167 @default.
- W2034333708 cites W2154672319 @default.
- W2034333708 cites W2167635287 @default.
- W2034333708 cites W2170118120 @default.
- W2034333708 cites W2186043533 @default.
- W2034333708 cites W3037873477 @default.
- W2034333708 cites W3098616803 @default.
- W2034333708 cites W3103820249 @default.
- W2034333708 cites W3104722657 @default.
- W2034333708 cites W4245661802 @default.
- W2034333708 cites W68413997 @default.
- W2034333708 doi "https://doi.org/10.1086/307350" @default.
- W2034333708 hasPublicationYear "1999" @default.
- W2034333708 type Work @default.
- W2034333708 sameAs 2034333708 @default.
- W2034333708 citedByCount "41" @default.
- W2034333708 countsByYear W20343337082014 @default.
- W2034333708 countsByYear W20343337082015 @default.
- W2034333708 countsByYear W20343337082016 @default.
- W2034333708 countsByYear W20343337082018 @default.
- W2034333708 countsByYear W20343337082019 @default.
- W2034333708 countsByYear W20343337082021 @default.
- W2034333708 countsByYear W20343337082022 @default.
- W2034333708 crossrefType "journal-article" @default.
- W2034333708 hasAuthorship W2034333708A5000945647 @default.
- W2034333708 hasAuthorship W2034333708A5012069547 @default.
- W2034333708 hasAuthorship W2034333708A5029607045 @default.
- W2034333708 hasAuthorship W2034333708A5051018099 @default.
- W2034333708 hasAuthorship W2034333708A5089400895 @default.
- W2034333708 hasBestOaLocation W20343337082 @default.
- W2034333708 hasConcept C121332964 @default.
- W2034333708 hasConcept C125857072 @default.
- W2034333708 hasConcept C1276947 @default.
- W2034333708 hasConcept C150846664 @default.
- W2034333708 hasConcept C190841160 @default.
- W2034333708 hasConcept C43481613 @default.
- W2034333708 hasConcept C44870925 @default.
- W2034333708 hasConcept C50425793 @default.
- W2034333708 hasConcept C555520305 @default.
- W2034333708 hasConcept C62520636 @default.
- W2034333708 hasConcept C68271606 @default.
- W2034333708 hasConcept C74902906 @default.
- W2034333708 hasConcept C8865038 @default.
- W2034333708 hasConcept C98444146 @default.
- W2034333708 hasConceptScore W2034333708C121332964 @default.
- W2034333708 hasConceptScore W2034333708C125857072 @default.
- W2034333708 hasConceptScore W2034333708C1276947 @default.
- W2034333708 hasConceptScore W2034333708C150846664 @default.
- W2034333708 hasConceptScore W2034333708C190841160 @default.
- W2034333708 hasConceptScore W2034333708C43481613 @default.